The 100-month Swift catalogue of supergiant fast X-ray transients - I. BAT on-board and transient monitor flares

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Table 5

BAT orbital periods adopted for Figs. 5 and 6.

Name	P_orb^a	Epoch
	(d)	(MJD)

IGR J16328−4726	10.076^b ± 0.065	54 256.08^b
IGR J16418−4532	3.73886^c ± 0.00003	53 560.2^c
IGR J16465−4507	30.258 ± 0.009	54 172.4236^d
IGR J16479−4514	3.31935 ± 0.00003	54 170.20^d
XTE J1739−302	51.47^e ± 0.02	52 698.2^e
IGR J17544−2619	4.93 ± 0.07	52 702.9^d
SAX J1818.6−1703	29.99 ± 0.08	52 712.3^d
AX J1845.0−0433	5.67^f ± 0.06	52 708.4397^f
IGR J18483−0311	18.56 ± 0.07	52 770.6^d

Notes.

^(a)

P_orb derived from standard folding analysis unless otherwise specified; errors on P_orb estimated from a Gaussian fit of the peak centroid.

^(b)

^bCorbet et al. (2010).

^(c)

Levine et al. (2011).

^(d)

Epoch of X-ray maximum.

^(e)

Drave et al. (2010).

^(f)

Goossens et al. (2013).

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